Videos and Simulations from the YouTube channel of Computational Science Zurich.

Videos and simulations of a network framework of cultural history, by COSS team, ETHZ.

Videos and simulations from the areas of fluid mechanics, nanotechnology and life sciences, by CSE Lab, ETHZ.

Time sequence of the formation of galaxy simulated with the RAMSES computational astrophysics code, by Prof. Ben Moore, CTAC, UZH.

The History of universe in 24 hours, by Ben Moore, UZH.

Geodynamo: Streamlines of flow of the liquid metal in the Earth's-like dynamo, Earth and Planetary Magnatism Group, ETHZ.

Milk 67 & Professor Ben Moore, University of Zurich

Geodynamo: A vortex containing strong magnetic field is formed on the axis of rotation, by EPM, ETHZ

Geodynamo: Streamlines of the magnetic field produced in the Earth's-like dynamo, by Earth and Planetary Magnetism Group, ETHZ.

Merger trees from numerical simulations of the origin of the Earth-Moon system, by Prof. Ben Moore, CTAC, UZH.

by Prof. Remi Abgrall, Mathematics, UZH.

Flows driven by precision in planetary cores, by EPM, ETHZ.

Precession driven dynamo (laminar regime): Isosurfaces of magnetic field strength (left) and velocity magnitude (right), by EPM, ETHZ.

Unstable regime: Isosurfaces of magnetic field strength. Insulating boundary conditions (left), conducting boundary conditions (right), by EPM, ETHZ.

Image by Prof. Eleni Chatzi, Institute of Structural Mechanics, ETHZ.

By Professor Ben Moore, UZH.